"Can life develop on an earth-sized moon of a jovian planet that orbits in the habitable zone of its parent star's system?"
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Silicate Mineralogy on Mars Indicates Wet Past
August 27, 2008 / Posted by: Daniella Scalice
Using data from the CRISM instrument on NASA’s Mars Reconnaissance Orbiter, astrobiologists from NAI’s SETI Institute and Marine Biological Laboratory teams present findings of silicate mineralogy indicating a wide range of past aqueous activity in the Mawrth Vallis on Mars. This work, published in the August 8 issue of Science, suggests that abundant water was once present on Mars and that hydrothermal activity may have occurred. The Mawrith Vallis could be a landing site for future rover missions to Mars.
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